Table 4.
Fraction of the CIB resolved into individual sources in our A3COSMOS and A3GOODSS databases.
| ALMA Band | Stotal, ALMA | Stotal, COBE | Percentage |
|---|---|---|---|
| [Jy deg−2] | [Jy deg−2] | resolved | |
| Band 3 ( * ) |
 |
2.2 ± 1.1 |
 |
| Band 4 |
 |
5.5 ± 2.6 |
 |
| Band 6 |
 |
19.1 ± 8.2 |
 |
| Band 7 |
 |
36.3 ± 14.8 |
 |
Notes. Total flux density per unit area inferred from A3COSMOS and A3GOODSS number counts and CIB emission measured with COBE (Fixsen et al. 1998) for ALMA Bands 3 (2998 μm), 4 (2082 μm), 6 (1233 μm), and 7 (925 μm). The last column gives the fraction of the CIB that is resolved into discrete sources using our number counts. ( * )Band 3 estimates for COBE are an extrapolation as they lie outside of the data range constrained in Fixsen et al. (1998).
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